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Citation for the original published paper (version of record):
Dolbin, A., Esel'son, V., Gavrilko, V., Manzhelii, V., Vinnikov, N. et al. (2011)
Quantum phenomena in the radial thermal expansion of bundles of single-walled carbon nanotubes doped with
3He. A giant isotope effect.
Low temperature physics (Woodbury, N.Y., Print), 37(6): 544-546 http://dx.doi.org/10.1063/1.3624780
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A. V. Dolbin
1, V. B. Esel'son
1, V. G. Gavrilko
1, V. G. Manzhelii
1, N. A.Vinnikov
1, S. N.
Popov
1, B. Sundqvist
2.
1
B. Verkin Institute for Low Temperature Physics & Engineering NASU, Kharkov 61103, Ukraine
2
Department of Physics, Umea University, SE - 901 87 Umea, Sweden Electronic address: dolbin@ilt.kharkov.ua
Quantum phenomena in the radial thermal expansion of bundles of single-walled carbon nanotubes doped with
3He. A giant isotope effect
PACS: 65.60.+a, 65.80.-g, 65.40.De, 64.70.Tg Abstract
The radial thermal expansion α
rof bundles of single-walled carbon nanotubes saturated with
3He up to the molar concentration 9.4% has been investigated in the temperature interval 2.1—9.5 K by high-sensitivity capacitance dilatometry. In the interval 2.1—7 K a negative α
rwas observed, with a magnitude which exceeded the largest negative α
rvalues of pure and
4He- saturated nanotubes by three and two orders of magnitude, respectively. The contributions of the two He isotope impurities to the negative thermal expansion of the nanotube bundles are most likely connected with the spatial redistribution of
4He and
3He atoms by tunneling at the surface and inside nanotube bundles. The isotope effect turned out to be huge, probably owing to the higher tunneling probability of
3He atoms.
keywords: Radial thermal expansion, single-walled carbon nanotube, helium, quantum effects, isotope effects
Introduction
Since their discovery by Prof. Iijima in 1991 [1], carbon nanotubes (CNTs) have been attracting intense interest from scientists owing to their unique geometry and extraordinary physical properties. The very high length-to-diameter ratios and the capability of CNTs to form bundles of several tens or even hundreds of tubes make it possible to form low-dimensional, ordered impurity phases at the bundles' surfaces [2,3]. Such phases consist of impurity molecules or atoms forming one-dimensional chains in the intertube grooves or in the interstitial channels in the bundles. They can also form two-dimensional layers at the bundle surface. It has been found experimentally [4—7] that the radial thermal expansion coefficients α
rof nanotube bundles are negative in the region of liquid helium temperatures. Gas impurities usually suppress the magnitudes of these negative values of α
rand reduce the temperature region where they exist.
The
4He impurity is an exception: when
4He is introduced both the magnitude of the negative α
rvalues and the temperature region of the negative thermal expansion increase [7]. This effect was
attributed to a tunneling redistribution of the
4He atoms at the surface and inside CNT bundles. It
is known [8, 9] that the processes of tunneling gives a negative contribution to the thermal
expansion of a system. It is then reasonable to expect that saturation of CNT bundles with
3He
would enhance the above effect because the smaller masses of
3He atoms must increase the
probability of tunneling.
2
In the present work we have, therefore, investigated the radial thermal expansion of single- walled carbon nanotubes (SWNTs) saturated with
3He using the dilatometric method. The temperature interval studied was 2.1—9.5 K. As will be shown below, the experimental results verify our expectation that the addition of
3He should enhance the negative thermal expansion; in fact the effect is surprisingly large, two orders of magnitude larger than for
4He.
Experimental technique
The radial thermal expansion of
3He saturated CNTs was investigated using a high- sensitivity low-temperature capacitance dilatometer with 2·10
-9cm resolution. The technique and the experimental apparatus are presented in detail elsewhere [10]. The sample was a cylinder 7.2 mm high and 10 mm in diameter, obtained by compressing a stack of thin (≤ 0.4 mm) plates consisting of in-plane oriented CNTs at 1.1 GPa. The plates were prepared by compressing (1.1 GPa) small amounts of CNT powder (Cheap Tubes, USA, CCVD method). It is known [11] that such pressure treatment of a thin CNT layer leads to a preferred orientation where the CNT axes mainly lie in the plane perpendicular to the applied pressure, the average deviation being about 4º. The alignment of CNT axes in the plane makes it possible to investigate preferentially the radial component of the thermal expansion of the tubes [12] and the effect of gas saturation upon the radial thermal expansion of SWNT bundles [4—7].
Just before starting the investigation, the cell with a pure CNT sample was evacuated at room temperature for 72 hours to remove possible gas impurities. It was then cooled to 2.1 K and a series of control measurements was performed. The results showed that the thermal expansion of the sample coincided, within the experimental error, with the values obtained previously for pure CNTs [12] (see Fig. 1a, curve 4).
3He gas was then fed to the measuring cell at T = 2.1 K.
The
3He was added in small portions as some quantities were sorbed by the nanotubes. This permitted us to maintain the pressure in the cell several times lower than the pressure of saturated
3He vapor at this temperature (151.112 Torr at T = 2 K [13]). The total amount of
3He absorbed by the pure CNT sample was 9.4 mol. % (94
3He atoms per 1000 C atoms). At this impurity concentration we were able to compare our results on the thermal expansion of the
3He- SWNT with those from previous measurements of the radial thermal expansion of CNTs saturated with
4He to the molar concentration 9.4% [7]. After the sorption was completed, an equilibrium of ~ 1·10
-4Torr was set in the measuring cell. Since the rise of the sample temperature in the course of measuring α
rcould entail some
3He desorption from the sample, the reproducibility of the results was checked at regular intervals by heating and subsequently cooling the sample by ΔT, where ΔT = 0.3 ... 1 K. If the results obtained under this cycling coincided, within experimental error, the effect of He desorption was regarded as negligible and the data were considered to be obtained in equilibrium. The absence of reproducibility was believed to show that at this and higher temperatures the desorption of the
3He impurity from the sample had some effect on the thermal expansion. The measurement was then stopped. Note that for the radial thermal expansion of the
3He-SWNT the data were observed to be reproducible in the interval T = 2.1—9.5 K, but no longer reproducible when cooling the sample to 9.7 K. When reproducibility was no longer observed the sample was heated to T = 11 K and held at this temperature under dynamic evacuation until an equilibrium pressure of 7.5·10
-2Torr was achieved in the system. During this process, a fraction of the
3He impurity was desorbed from the sample. The sample was then cooled back down to the lowest temperature, 2.1 K, and the radial thermal expansion was measured again.
Results and discussion.
The temperature dependence of the radial thermal expansion coefficient α
rof the
3He-
SWNT system is shown in Fig. a. Solid circles represent α
rof the sample with the initial
3He
concentration 9.4 mol. %, empty circles data for the same sample after partial removal of the
3He
impurity by heating at 11 K. The inset in Fig. a shows the low-temperature data for the partially
evacuated sample on an expanded scale to enable a comparison with earlier studies, while Fig. b is shown on an intermediate scale for further comparisons with the saturated sample.
2 3 4 5 6 7 8 9 10 11
-20 -15 -10 -5 0 5
2.0 2.5 3.0 3.5 4.0 4.5 -0.2
0.0 0.2 0.4 0.6
10-6 K-1
T, K 1 2
4 3 2 3
r 10
-6K
-1T, K
1
4
a)
2.2 2.4 2.6 2.8 3.0 3.2 3.4
-6 -5 -4 -3 -2 -1 0
2,3,4
r 10
-6K
-1T, K
1